Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-03T01:31:21.221Z Has data issue: false hasContentIssue false
  • English
  • Français

Dust Near the Nucleus of M 31

Published online by Cambridge University Press:  14 August 2015

Hugh M. Johnson
Hugh M. Johnson*
Affiliation:
Lockheed Missiles and Space Company, Palo Alto, Calif., U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Special photographic observations reveal silhouetted dust patterns as close as 6″ from the nucleus. The spatial distribution and kinematics of the dust are discussed.

Type
Part V Distribution of Dust and Gas
Information
Symposium - International Astronomical Union , Volume 52: Interstellar Dust and Related Topics , 1973 , pp. 215 - 217
Copyright
Copyright © Reidel 1973 

References

Baade, W.: 1958, in O'Connell, D. J. K. (ed.), Stellar Populations , North-Holland Pub. Co., Amsterdam, p. 3.Google Scholar
Baade, W.: 1963, in Payne-Gaposchkin, C. (ed.), Evolution of Stars and Galaxies , Harvard Univ. Press, Cambridge, p. 59.Google Scholar
Copeland, R.: 1886, Monthly Notices Roy. Astron. Soc. 47, 49.Google Scholar
Johnson, H. M.: 1961, Astrophys. J. 133, 309.CrossRefGoogle Scholar
Johnson, H. M. and Hanna, M. M.: 1972, Astrophys. J. Letters 174, L 71.Google Scholar
Kinman, T. D.: 1965, Astrophys. J. 142, 1376.Google Scholar
Pooley, G. G. and Kenderdine, S.: 1967, Nature 214, 1190.CrossRefGoogle Scholar
Rubin, V. C. and Ford, W. K. Jr.: 1971, Astrophys. J. 170, 25.Google Scholar
Spinrad, H.: 1971, in O'Connell, D. J. K. (ed.), Nuclei of Galaxies , North-Holland Pub. Co., Amsterdam, p. 45.Google Scholar